Projection apparatus for a small planetarium



PROJECTION APPARATUS FOR A SMALL PLANETARIUM Oct. 31, 1939.

E. UNGLAUBE El' AL Filed Dec. 20, 1937 2 She ets-Sheefc 1 Oct. 31, 1939. E. UNGLAUBE ET AL 2,178,352

PROJECTION APPARATUS FOR A SMALL PLANETARIUM Filed Dec. 20, 1937 2 Sheets-Sheet 2 9- 216 yd 2/e 22a W m m: 47

v30 4 is a op p V ew On t unit consisting of the sheet metal sphere I a a ball-shaped source 30 UNITED STATES PATENT OFFICE PROJECTION APPARATUS FOR A SMALL PLANETARIUM Emil Unglaube and Georg Kiehlmann, Glogau,

Germany Application December 20, 1937, Serial No. 180,797

In Germany July 9, 1937 .7 Claims. in. 88-24) This invention relates to a projection apparatus sphere. A bevel wheel III having ten teeth for a small planetarium. meshes with the toothed wheel I68 and is keyed f'he object of the invention is to provide a on the end of ashaft 2. The reference numerals universal planetarium which maybe used as asof the toothed wheels, pinions and bevel wheels 5 tronomical displaying instrument for public asare selected here and in the following description 5 tronomical' observatories, museums, fairs and so that they indicate at the same time the number other entertainments and as instructive teachof teeth. The shaft 2 is rotatably mounted in ing means for schools. With the aid of the proa bearing 2a fixed on the bottom platev lb of the J'ecting apparatus according to the invention the hollow sp e la d q ppe W a C k 1)- movement and the change of the luminous shape The bearing 2a is carried by a suitable frame. of the moon, of the annual circles of the sun, the In the drawings a tripod frame 20 is shown. The eclipses and the loop course of the planets are longitudinal axis of shaft 2 forms an angle of represented. v 23 with the ecliptic shaft I. If the axle Zis Other tasks and tests which are connected rotated, the ecliptic shaft I rotates in accordwith the construction, combination and arrangeance with the ratio of transmission of 1 to 366.24 15 ment of the individual elements will result from es as r pi y s this ratio being the following detailed description. termined by the wheels Ill, I68, 5 and I09. The i The invention is illustrated, by way of example, ratio of transmission is in the accompanying drawings, in which:

go Fig. 1 is a total view of the projection appa- =366.24 I

ratus in strongly reduced scale and partly in 10 5 section. If the hollow sphere Ia is turned, that is if the Fi 2 is a top plan view n s c Of the upper whole apparatus is turned 366.24 times, and the part of the projection apparatus shown in Fig. 1. crank 2 with wheel III is held, around which 25 The scale of 2 is e e t a t e Sc e of wheel I68 circulates, the ecliptic shaft rotates 25 i 1. once and in opposite direction, it carries out F 3 is a cross-section through the m therefore only 365.24 rotations (366.241= p c or which formapa t of thedevice shown 3s5.24='1 earth year). On the portion of the n F ecliptic shaft I projecting from the upper part of the Mercury-proje r nd f th V n s-P of light 3 is fixed, mounted in a set 011 portion of J'ector which form part of the device shown i the ecliptic shaft so that the source of light is standing accurately in the axis of rotation of the ig- 5 i e s ti on line V of h ecliptic shaft. The half of the incandescent pr l s p p r being n hown for deafness lamp 3 facing the-ecliptic shaft is blackened, so 35 selke-v I that the light rays can radiate only towards the e p c pp shown in e side which is remote from the set off portion ings is employed in conjunction with a spherical Id. The source of light 3 is the moon-lttmp" projection wall, and the apparatus is mounted in of the moon-projector I2.

40 t Centre O the P j l l he p o The moon-projector consists of a tube I2 which 40 ection cupola is not shown as its construction i closed t n end by alien with prisms I21: d p y en i kn wn o anyone skilled-in and at the other end by an opaque plate IN). the Within the tube I2 a glass pane I3 is fixed with On the lower end of shaft -I, which will. be the aid of a carrying arm I3a so that this glasshereinafter called ecliptic shaft a. toothed pane comes, relative to the moon-lamp 3, into 45 wheel I09 is fixed whichhas a hundred and nine the rays radiating from the same when tube I2 teeth with which a pinion 5'meshes which has is in-according position. The face, that is five teeth. The pinion 5 is keyed on a shaft the spot-picture of the moon, is painted on pane 5a which is rotatably mounted in a bottom plate I3 as really seen from the earth. The tube I2 my ID of a hollow sheet metal sphere flattened at is arranged so that it can loosely rotate on the the upper end and at the lower end. On the ecliptic shaft I and so that the angle which the. shaft 5a a toothed wheel I68 having one hundred longitudinal axis of tube I2 forms with shaft sixty eight teeth is keyed. The ecliptic shaft I I can change from to The tube I2 is extends through the sheet metal sphere Ia and is mounted in a fork by means of two lateral 55 rotatably mounted in the bottom plate lb of this pins I 2d so that it can swing around a transverse 55 axis, the fork being near the one end of tube I2. The fork I2c is fixed on the upper end of a sleeve I9a enclosing loosely rotatable the ecliptic shaft I, and one end of the same carries a toothed wheel I9. Two pins Iia and I5!) are fixed on the lower end of the tube I2 and support said tube I2 upon a plate I6. This plate has a bore through which the sleeve-like hub I9a of the toothed wheel I9 freely extends. The plate I6 is constructed and fixed on the upper end of the sleeve-like hub of a toothed wheel 62 so that the surface of plate I6 forms an angle of 85 with the axis of rotation of the ecliptic shaft. If the eclipticshaft I is standing vertical, the upper side of plate I6 forms with the horizontal plane an angle of 5' (measured in downward direction) this angle corresponding to the inclination of'the lunar orbit relative to the ecliptic. A box I4 is mounted on the upper side of tube I2, the wall of said box having a row I4a of holes. A source of light I4?) is arranged in the middle of box I4 so that therays from this source of light can pass through the holes of the row Ila towards the outer side.

The toothed wheel IS, on the hollow hub I9a of which the carrying fork I20 of the moonprojector I2 is fixed, is mounted between the cover plate Ic of the sheet metal sphere Ia and an intermediate plate Ie which is rigidly connected with the top plate by a vertical bar If. Also the other wheels of the gear are mounted between the plates I and le, said gear transmitting the rotation of the ecliptic shaft I upon the toothed wheel I9. The gear consists of a toothed wheel 46 keyed on shaft I and of toothed wheels 26 and I21 keyed the one above the other on an intermediate shaft II. The toothed wheel2ll meshes with the toothed wheel 40, whereas the toothed wheel I21 meshes with the toothed wheel I9. The ratio of transmission between the ecliptic shaft and the toothed wheel amounts therefore to Therefore, if the ecliptic shaft has carried out a complete rotation, the toothed wheel I9 and the moon-projector connected with the same have carried out 13.3684 rotations about shaft I. This number of rotations corresponds accurately to the number of the moon circulations during an earth year.

To disc I6 another movement than that of the moon-projector I2 is imparted with the aid of a gear consisting of the toothed wheels 62, Illa. 36, 6, 20 and 40. The pinion I60. meshing with the toothed wheel 62 is keyed on the shaft 36a of toothed wheel 36, said shaft being journalled in the top plate Ic of the sheet metal sphere Ia. .The toothed wheel 36 meshes with the teeth of pinion 6, which is keyed on the above mentioned intermediate shaft II which is rotatably mounted in the plates lo and Ie. The toothed wheel 20 already mentioned, keyed on this intermediate shaft, meshes with the teeth of the toothed wheel 40 keyed on shaft I. The plate I6, which determines the inclination of the moon-projector I2 relative to shaft I, is therefore turned in accordance with the ratio of transmission of the above mentioned gear can turn around the ecliptic shaft I.

of the ecliptic shaft I carries out only 0.0537 rotation. The plate I6 consequently stands almost still during a complete rotation of the ecliptic shaft I. 18.6 rotations of shaft I are required to once rotate the plate around the ecliptic shaft. This illustrates, how the points of intersection of ecliptic and lunar orbit wander, owing to the shifting of the latter in l8.6 years round through the ecliptic.

For illustration of the eclipse of the sun a diaphragm I8 is fixed on the tube I2 of the moon-projector and gets into the path of rays 4a of the sun-projector 4 at the two points in which the moon course is in the height of the ecliptic.

The sun-projector 4 consists of a tube which is open only at one end and carries on this end an arm 4b. This arm 4b is mounted on the one side of a sleeve 40 through which the ecliptic shaft I extends. The sleeve 4c is rigidly connected with the ecliptic shaft I by means of clamping screws id. The open end of the sunprojecor has a lens 4e and a prism 4g, opposite which a spherical source of light 4 is arranged (the sun-lamp). The arrangement is'therefore such that the light rays radiating from the sunprojector pass at .he side of the ecliptic shaft I The sun-projector turns, together with the ecliptic shaft I, that is carries out an annual move ment.

A circular disc 9a serves for representing the lunar eclipse and is fixed on a wire 9 so that it can get into the path of rays of the moonprojector I2. The wire 9 is fixed on the ecliptic shaft I and therefore participates in the (annual) movement of the same. The circular disc 9a corresponds to the cross-section of the earth shadow and prevents in its effective position, that the light rays of the lunar-projector impinge onto the projection wall.

Beneath the moon-projector the Mars-projector I1 is arranged which consists of a tube II, a source of light I'Ia and an optic system the latter being composed of a lens and of a prism. The tube I1 is fixed on a rod IIc so that it forms the extension of this rod. The rod He is mounted, with the aid of a sleeve IId, freely rotatable on the hollow hub 62a of the toothed wheel 62 so that the Mars-projector IT The Marsprojector is driven fromthe already mentioned intermediate shaft II which, with this object in view, is equipped with a toothed wheel 25. This toothed wheel is in mesh with a toothed wheel 94 which is mounted on the hollow hub 62a of the toothed wheel 62 so that it can loosely rotate on this hollow hub. A bar 94a is fixed on the toothed wheel 94 so that its end projects beyond the circumference of wheel 94. In this projecting portion of bar 94a the pivot axle of a toothed wheel 50 isjournaled which meshes with the toothed wheel 40a. The latter toothed wheel is keyed on the hub 62a of the toothed wheel 62 and therefore rotates very slowly, together with the carrying plate I6 of the moon-projector I2. The wheel 56 has an eccentric pin I90 engaging in a longitudinal slit of rod I'Ic.

The toothed wheel 84 is driven from the ecliptic shaft I at a ratio of transmission of The Mars-projector turns therefore approximate- 1y half as rapidly as the ecliptic shaft I. This fstandstill'durlng one rotation of the ecliptic jecto'ri il with the aid of theeccentric, gear I90v lagging of the movement -of the Mars I wheel-.tirelatlve to the rotation oi', the ecliptic shaft. I, has the result,;that the, toothed wheel 1 50-. rolls on the toothed wheel 40a, thelatter, as mentioned above, turning accurately, as slowly 'as plate 16, that is being practically almost at "shaft; I Consequently, afreciprocating' movement corresponding to the geocentric movement'of the planet Mars is communicated tothe Mars proateverycomplete rotation of the ecliptic shaft I. /The'Mercury-'p rojector I! and the Venus-projecto'r I02 are arranged .above the Sun-projector.

4. Each'projector consists of a tube I 0I, respectively I02 with anioptical system IOIa, I020. re-

spectively, composed of lens and prism and with an incandescent lamp, IOIb, I02b respectively.

' 0n the ecliptic shaft a transverse head I03.is.

fixed, at'the ends of which arms I03a,j I03b re- H spectively, each. at the same distance from the ecliptic shaft I, are arranged 0n the lower side of each arm a pin I03c, I03d respectively is fixed,

respondingcarrying rod. A toothed wheel 20a is arranged on the transverse head I03, the axle 20b of this toothed wheel beingjournaled in a bore extending through the point of intersection of the; central longitudinal axis of the transverse head I03 withthecentral longitudinal axis of the arm NM. .The lower end of the shaft 20b projecting from the lower side of the transverse head carries an arm 200, the free end of which carries a bearing enclosing the rod I04. The toothed wheel 2.0a meshes with a toothed wheel which is arranged on the ecliptic shaft I, but

. not keyed on the same, but fixed on a bar lg.

This bar forms part of the supporting frame consisting of the above mentioned plates lb, lo, Ie, If.

The rod I of the Venus-projector extends W, Lu)

through a bearing 40d,.which is arranged on the endof-an arm 40c. This arm is fixed on the shaft 40e-which is rotatably mounted so that it can turn in a bore of the transverse head I031 and-is connected with a toothed wheel 40b at its upper end projecting over the transverse head. The axis of rotation of the shaft 40c is in the point of intersection of the central longitudinal axis of the transverse head I03 with the central longitudinal axis of the arm I031). The toothed wheel 40b meshes with the toothedwheel 25a, which is keyed on the lower-side of the toothed wheel 63 and has a central bore through which the ecliptic shaft I extends. The toothed wheels 25a and 03 are therefore stationary and do not participate inthe rotation of the ecliptic-shaft I,

The rotation of the ecliptic shaft I is transmitted with the aid of the transverse head I03,

the arms I03a and I00!) and the rods I04, I05,,

upon thetwo projectors for Mercury and Venus, so that both projectors participate in the annual" movement of the ecliptic shaft l To every projector, however, an additional oscillating movement around the pins I030, I03d respectively iseimparted, and this movement-is produced by the rolling of'the toothed wheels a and 40?) on the stationary toothed .wheels 63 and 250 At every completerotation of the ecliptic shaft I the toothed wheel 20a rotates 3.15tim'es around seems it s movedby the transverse head m once around thestationarytoothed wheel This self-rotation of the toothed wheel -20a has the result, that the Mercury-projector IOI during a complete rotation of the ecliptic shaft is oscillated 3.15 times to and fro around the" pin I030. The same sto be said'for theVenus-projector. .which accor g to theratio of transmission of the toothed wheels a andb oscillates to and fro, around the pin I03d, 0.625 time during a complete rotation of the eclipticshaft. a

On the upper side of the bar la a toothed wheel 24 is fixed, through the central bore of which the ecliptic shaft I extends. Above this stationary toothed wheel 24 an arm I rigidly connected with the ecliptic shaft I is arranged, the endof which,

projecting beyond the circumference of the toothed wheel 24 carries an auxiliary shaft la. On this auxiliary shaft, which extends through the arm I, three toothed wheels are keyed, of which the one, 24a, is arranged below arm I and meshes with thestationary toothed wheel 24. The two toothed wheels 51 and 54 arranged above the arm I and keyed on the shafttla arerigidly connected the one with the other. The toothed wheel 54 meshes with a toothed wheel 59a which. is mounted onthe ecliptic shaft so that it can loosely rotate around this shaft. The hollow hub 59b of the toothed wheel 59 extends through a corresponding central bore of the'toothed wheel 59a. A hollow cylinder 21' is fixed on the toothed Wheel 5911 and has an aperture in its wall. From this aperture extends a tube 2 la, in the open right hand end of which an optical system 2") is mounted which is composed of a lens and of a prism; this device forms the Jupiter-projector.

The hollow cylinder 2I is closed at its lower end,

. whereas its upper end is open. In upward ,direc-' tion follows on the hollow cylinder 2I a hollow cylinder 2Ic, the lower side of which is open, whereas its upper side has a cover, that is is closed. The'hollow cylinder 2|.c carries the Saturn-projector which consists of a tube 2 Id-with an optical formed by the hollow cylinders 2i and 2Ic an incandescent lamp 8 is located which is fixed on one side of the ecliptic shaft I so that its light rays can project as well through the Jupiterprojector' as through theSaturn-proje'ctor. The

lamp 8 participates in the annual movement of the ecliptic shaft I. The same is valid for the arm I which rotates the auxiliary shaft Ia with the'toothed wheels 24a, 51 and 54 fixed thereon.

4 As, however, the toothed wheel 24a meshes with the toothed wheel 24 which is stationary, that is, does not participate in'the rotation of the ecliptic shaft I, a common self-rotation is imparted to the toothed wheels melt and 54 which almost completely holds back the co ter wheels 59 and I h a complete rotation of the ecliptic shaft i the wheel 59 rothe intermediate shaft la therefore annuls for the greatest part the annual movement of the toothed wheels 59 and 58a so that the Jove-projector and the Saturn-projector move only very little during one complete rotation of the ecliptic shaft I. The two projectors are now outrun by the source of light 8 annually on a narrower circle. Consequently, the planets-picture formed by the projectors lib and 2 Id on the projectioncupola oscillates back parallactically. The planets-picture alters, owing to the slightly differentiating distance of lamp and lens, slightly as regards its size so that, besides the retrograde movement also the apparent alteration of size of the planets Jove and Saturn is shown.

In order to represent further for all five planets also the alteration of brightness which is produced by the annual course of the sun, a hollow cylinder 22 of transparent material islfixed, with the aid of the transverse head 22a, on the ecliptic shaft I so that it encloses all projectors. By blackening the transparent cylinder 22 within the area of the rays from the individual projectors it is possible to accordingly screen off the planets-pictures.

The sheet metal sphere la is perforated, so that the rays of the incandescent lamp lh arranged in the middle of the sheet metal sphere passing through these holes, draw upon the not shown projection cupola the picture of the starry sky in the form of light spots. The lamp In is arranged in a set off part Ii of shaft I so that it is in the central longitudinal axis of the ecliptic shaft i.

We claim:

1. A projection apparatus fora small planetarium comprising in combination a hollow spherical body perforated to simulate the position of the fixed stars, a main shaft extending through the centre of said spherical body, a stand rotatably supporting said spherical body at a-point eccentric to said main shaft, a short shaft extending through the'point of support into said spherical body at an angle to said main shaft, means for turning said short'shaft to rotate said spherical body, a reduction gear between said short shaft and the lower end ofsaid main shaft to rotate said shaft at a lower speed than said spherical body, a source of light'on said main shaft in the centre of said main shaft projecting its rays through the perforations in said spherical body, a plurality of projectors, each presenting a celestial body movably mounted on the upper end of said main shaft, one above the other, gears connecting each of said projectors to said main shaft to impart different movements to said projectors :during the rotation of said main shaft, a source of light in each of said projectors, and a frame extending through and carrying said spherical body and said gears and supporting said main shaft at its top and bottom ends.

2. A projection apparatus'for a small planetarium, comprising in combination a hollow spherical body perforated to simulate the position of the fixed stars, a main shaft extending through the centre of said spherical body, a stand rotatably supporting said spherical body at a point eccentric to said main shaft, a short shaft extending through. the point of support into said spherical body at'an angle to said main shaft, means for turning-said short shaft to rotate said spherical body, a reduction. gear between said short shaft and the lower end of said main shaft to rotate said shaft at a lower speed than said spherical body, a source of light on said main shaft in the centre of said main shaft projecting its rays through the perforations in said spherical body, a plurality of projectors each representing a celestial body movably mounted onthe upper end of said main shaft, one above the'other, gears connecting each-of said projectors to said main shaft to impart diflerent movements to said projectors during the rotation of said main shaft, a source of light in each of said projectors, one of said projectors representing the moon comprising va sleeve rotatable on said main shaft, a pair of arms projecting from said sleeve, a projector tube oscillatably carried by said sleeve and having diametrically opposite bores for the free passage of said main shaft, a lens at the front end of said tube, the, source of light in the projector arranged towards the rear'end of the tube and rigidly mounted on and rotatable with said main shaft and comprising a bulb blackened on one side to intermittently project its rays through said lens, the gear of this projector comprising a plurality of gear wheels, a wedge-shaped disc rigidly mounted on one of said gear wheels concentric with said main shaft, and pins projecting downwards from the under side of said tube and bearing against said disc to vary the inclination of said tube during the rotation of said shaft and saidgears.

3. A projection, apparatus for a small planetarium, comprising in combination a hollow spherical body perforated .to simulate the position of the fixed stars, a main 'shaft extending through the centre of said spherical body, a stand rotatably supporting said spherical body at a point eccentric to said main shaft, a 'short shaft extending through the point-of support-into said spherical body at an angle to said main shaft, means for turning said short shaft to rotate said spherical body, a reduction gear between said short shaft and the lower end of said main shaft to rotate said shaft at a lower speed than said spherical body, a source of light on said main shaft in the centre of said main shaft pro-' jecting its rays through the perforations in said spherical body, a plurality of projectors each representing a celestial body movably mounted on the upper end of said main shaft, one above the other, gears connecting each of said projectors to said main shaft to impart different movements to said projectors during the rotation of said main shaft, a source of light in each of said projectors, one of said projectors representing the moon, comprising a bracket. loosely mounted on said main shaft, a projector tube closed at its rear end and oscillatably mounted on said bracket tube, means for oscillating said tube during the rotation of said main shaft, a lens on the front end of said tube, the source of light of the projector rigidly mounted on said main shaft towards the rear end of said tube, and a pane of glass arranged In said tube between said lens and said source of light and carrying a transparent picture corresponding to the spot pictureofthe moon.

4. A projection apparatus for a small planetarium, comprising in combination a hollow spherical body perforated to simulate the position of the fixed stars, a main shaft extending through the centre of said spherical body, a stand rotatably supporting said spherical body at a point eccentric to said main shaft, a short shaft extending through the point of support into said spherical body at an angle to said main shaft, means for turning said short shaft to rotate said spherical body, a reduction gear between said short shaft and the lower end of said main shaft to rotate said shaft at a lower speed than said spherical body, a source of light on said main shaft in the centre of said main shaft projecting its rays through the perforations in said spherical body, a plurality of projectors each representing a celestial body movably mounted on the upper end of said main shaft, one above the other, gears connecting each of said projectors to said main shaft to impart different movements to said projectors during the rotation of said main shaft, a source of light in each of said projectors, one of said projectors representing the sun comprising a tube closed at its rear end and mounted at its front end on the main shaft, an opticar system at the front end of said tube, a source of light at the rear end of said tube projecting a beam of light through said optical system, and a screen on one of the other projectors adapted to be brought intermittently into the beam of light projected through said optical system.

5. A'projection apparatus for a small planetarium, comprising in combination a hollow spherical body perforated to simulate the position of'the fixed stars, a main shaft extending through the centre of said spherical body, a stand rotatably supporting said spherical body at a point eccentric to said main shaft, a short shaft extending through the point of support into said spherical body at an angle to said main shaft, means for turning grid short shaft to rotate said spherical bodyf a reduction gear between said short shaft and the lower end of said main shaft to rotate said shaft at a lower speed than said spherical body, a source of light on said main shaft in the centre of said main shaft projecting its rays through the perforations in said spherical body, a plurality of projectors each representing a celestial body movably mounted on the upper end of said main shaft, one above the other, gears connecting each of said projectors to said main shaft to impart different movements to said projectors during the rotation of said main shaft, a source of light in each of said projectors, three of said projectors representing the Mars, Mercury and Venus respectively and each.

comprising a projector tube closed at one end, a lens at the other end of said tube, and an incandescent lamp in said tube and projecting a beam-of light'through said lens, circulating gears, one connecting each of said projectors to the main shaft, and rod systems one connected to the tube of each projector to impart a retrograde motion to said projectors during their circulating movement.

6. A projection apparatus for a small planetarium, comprising in combination a hollow spherical body perforated to simulate the position of the fixed stars, a main shaft extending through the centre of said spherical body, a stand rotatably supporting said spherical body at a point eccentric to said main shaft, a short shaft extending through the point of support into said spherical body at, an angle to said main shaft, means for turning said short shaft to rotate said spherical body, a reduction gear between said short shaft and the lower end of said main shaft to rotate said shaft at a lower speed than said spherical body, a source of light on said main shaft in the centre of said main shaft projecting its rays through the perforations in said spherical body, a plurality of projectors each representing a celestial body movably mounted on the upper end of said main shaft, one above the other, gears connecting each of said projectors to said main shaft to impart diflerent movements to said projectors during the rotation of said main shaft, a source of light in each of.said projectors, two of said projectors representing Jupiter and Saturn comprising a common casing freely rotatable about the main shaft and divided in horizontal direction into two halves, two parallel tubes one projecting from each half of said casing, two lenses one at the outer end of each of said tubes, a common incandescent lamp fixed on said main shaft in said casing and projecting a beam of light through both of said tubes, and a circulating gear connecting both of said casing halves to saidmain shaft to rotate said halves about said main shaft at different speeds.

7. A projection apparatus for a small planetarium, comprising in combination a hollow spherical body perforated to simulate the posi-' shaft extending through the point of support into said spherical body at an angle to said main shaft, means for turning said short shaft to rotate said spherical body, a reduction gear-between said short shaft and the lower end of said main shaft to rotate said shaft at a lower speed than said spherical body, a source of, light on said main shaft in the centre of said main shaft projecting its rays through the perforations in said spherical body, a plurality of projectors each representing a celestial body movably mounted on the upper end of said main shaft, one above the other, gears connecting each of said projectors to said main shaft to impart different movements to said projectors during the rotation of said main shaft, a source of light in each of said projectors, a cylinder of transparent material fixed on the upper end of the main shaft and extending around the projectors, said cylinder having a plurality of circular stripes blackened at different intensities, and each stripe arranged within the range of projection of one of said projectors.

EMIL UNGLAUBE. GEORG KIEHLMANN. 

